
#DEBUG
0		debug level
0		cpu to watch
10.0		dt between normal code output to stdout
F		usebarriers - forces the code to stop and wait more often

#RESTART
F

# -----------------------------------------------------------------------
#GRID
1	        lons
1	        lats
-90.0		minimum latitude to model
90.0		maximum latitude to model
0.0		longitude start to model (set to 0.0 for whole planet)
0.0             longitude end to model (set to 0.0 for whole planet)

#ALTITUDE
0.0		minimum altitude to use
300.0		maximum altitude to use (ignored unless the following is F)
F		use stretched grid

# -------------------------------------------------------------------------
#DIFFUSION
T
100.0		Eddy Diffusion Coefficient (Should be about 37.5 for 1-D runs)
0.020		Total Eddy Diffusion applied at alts below this pressures level
0.003		No Eddy Diffusion at altitudes above this pressure level

#THERMALDIFFUSION
2.22e-4		Thermal conductivity (code use kappa = number * T**0.75)

#PHOTOELECTRON
0.00       Efficiency of photoelectron heating

#NEUTRALHEATING
0.02       Efficiency of photoelectron heating

#THERMALCONDUCTION
5.6e-4     Thermal conductivity (o2)
7.6e-4     Thermal conductivity (o)
0.72       Thermal conductivity (^s)
# -------------------------------------------------------------------------

#TIMESTART
2002
03
18
00
00
00

#TIMEEND
2002
03
18
00
05
00

#AUSMSOLVER
T       	Use AUSM+-up Solvers

#CPUTIMEMAX
604800		Maximum amount of cputime to use before stopping the code

#SAVEPLOTS
7200.0		dt for writing restart files
2		how many output files do you want
3DALL		output style
7200		dt for output
3DUSR		output style
43200		dt for output

# ----------------------------------------------------------------------
#CFL
0.7		percentage of maximum allowable time-step to take

#LIMITER
mc		only limiter available
2.0

#LOGFILE
1.0		dt for output to a log file

# ----------------------------------------------------------------------
#STATISTICALMODELSONLY
F		if you want to run with msis and iri only (i.e. not GITM)
1800.0		time step to take if you run with msis and iri

#ELECTRODYNAMICS
60.0		how often to update potential
60.0		how often to update aurora and euv

#KP
1.0

#APEX
F		Use apex magnetic coordinate system

#AMIEFILES
none      northern hemisphere amie file
none      southern hemisphere amie file

# ----------------------------------------------------------------------
#DAMPING
T      Turn on vertical velocity damping term in vertical_solver

#DUST
0.5
0.003

#INITIAL
T               initialize thermosphere using MSIS
F               initialize ionosphere using IRI
100.0           if msis is false, then this is the temperature at the base
250.0           if msis is false, then this is the temperature at the top
140.0           if msis is false, then this altitude of the temperature change
20.0            if msis is false, then this width of the temperature change
1.17e18         CO2
4.03e15         CO
2.31e15         O
3.26e16         N2
2.00e20         O2
2.40e21         Ar
3.20e17         He

#F107
130		f10.7
130		f10.7 averaged over 81 days

#THERMO
T		 UseSolarHeating
F		 UseJouleHeating
F		 UseAuroralHeating
F		 UseNOCooling
T		 UseOCooling
T		 UseConduction
F		 UseTurbulentConduction

#VERTICALSOURCES
25.0

#TIDES
F		UseMSISOnly
F		UseMSISTides
F		UseGSWMTides
F		UseWACCMTides

#GSWMCOMP
F
F
F
F

(All false below is new model of EUV!)
EUVMODEL
F			UseEUVAC
F			UseTobiska
F			UseAboveHigh
F			UseBelowLow

#FORCING
T		UsePressureGradient
F		UseIonDrag
T		UseNeutralDrag
T		UseViscosity
T		UseCoriolis
T		UseGravity

#IONFORCING
F
F
F
F

#DYNAMO
F		UseDynamo
0		DynamoHighLatBoundary (if UseDynamo is T)
0		nItersMax (if UseDynamo is T)
0		MaxResidual (if UseDynamo is T)
0		IncludeCowling (if UseDynamo is T)
0		DynamoLonAverage (if UseDynamo is T)

#CHEMISTRY
T		UseIonChemistry
F		UseIonAdvection
T		UseNeutralChemistry

#STRETCH
65.0		! location of minimum grid spacing
0.0		! Amount of stretch 0 (none) to 1 (lots)
1.0		! More control of stretch ( > 1 stretch less < 1 stretch more)

#END
